Stellar mass functions in the peaks of the Hyperion protostructure at z~2.5 show a mass-dependent excess relative to the field, with ~10x enhancement at log(M*/M⊙)~11 versus ~3.5x at log(M*/M⊙)~9.5.
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Euclid early release observations of Abell 2390 yield consistent weak lensing mass estimates from three shape catalogs and tomographic bins after contamination corrections.
citing papers explorer
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The HST-Hyperion Survey: Environmental Imprints on the Stellar-Mass Function at z~2.5
Stellar mass functions in the peaks of the Hyperion protostructure at z~2.5 show a mass-dependent excess relative to the field, with ~10x enhancement at log(M*/M⊙)~11 versus ~3.5x at log(M*/M⊙)~9.5.
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Euclid: Early Release Observations. Weak gravitational lensing analysis of Abell 2390
Euclid early release observations of Abell 2390 yield consistent weak lensing mass estimates from three shape catalogs and tomographic bins after contamination corrections.